Geodesic
The stream of secondary particles in the circumlunar space
Vestnik Tomskogo gosudarstvennogo universiteta. Matematika i mehanika, no. 4 (2011), pp. 131-133

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A mathematical model which permits one to calculate a circumlunar cloud of secondary particles by a known meteorite stream on the Moon surface is considered. The cloud characteristics in the sphere of the Moon gravitation are presented. The article gives a review of works executed on the Calculus Department of Tomsk State University in 1977–80.
Keywords: primary meteoroid stream, cratering, secondary particles stream, size, velocity, energy of particles.
Mots-clés : mass 
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     author = {E. N. Krivyakova},
     title = {The stream of secondary particles in the circumlunar space},
     journal = {Vestnik Tomskogo gosudarstvennogo universiteta. Matematika i mehanika},
     pages = {131--133},
     publisher = {mathdoc},
     number = {4},
     year = {2011},
     language = {ru},
     url = {http://geodesic.mathdoc.fr/item/VTGU_2011_4_a15/}
}
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E. N. Krivyakova. The stream of secondary particles in the circumlunar space. Vestnik Tomskogo gosudarstvennogo universiteta. Matematika i mehanika, no. 4 (2011), pp. 131-133. http://geodesic.mathdoc.fr/item/VTGU_2011_4_a15/